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Nuclear Symmetry Energy from a Relativistic Mean Field Theory |
| OUYANG Fei, LIU Bei-Bei, CHEN Wei** |
Department of Physics, Jinan University, Guangzhou 510632
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| Cite this article: |
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OUYANG Fei, LIU Bei-Bei, CHEN Wei 2013 Chin. Phys. Lett. 30 092101 |
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Abstract We discuss the density dependence and coupling-constant dependence of the nuclear symmetry energy in the relativistic mean field approximation of the σ?ω?ρ model. An extremely stiff density dependence of symmetry energy is obtained. At the same time, we find that the coupling constants gσ and gω have greater effect on the nuclear symmetry energy than the self-coupling constants c and d. In particular, gω and gσ determine the slope L and curvature Ksym of nuclear symmetry energy at saturation density, respectively.
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Received: 07 May 2013
Published: 21 November 2013
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